Other
Scientific paper
Jul 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mpia.rept.....l&link_type=abstract
Final Report, Dec. 1981 Max-Planck-Inst. für Aeronomie, Katlenburg-Lindau (Germany, F.R.).
Other
Data Processing, Helios A, Helios B, Zodiacal Light, Data Reduction, Interplanetary Dust, Milky Way Galaxy, Spatial Distribution
Scientific paper
The method used to derive the spatial distribution of interplanetary dust and the results are presented. A complete list of literature, concerning this experiment, is included. The radial gradients of the spatial distribution, and the node and inclination of the symmetry plane of interplanetary dust are reliably determined. Zodiacal light is remarkably constant and variations other than these caused by the Helios orbital motion were not observed. Data on light intensity and polarization of the Milky Way Galaxy were also obtained.
Almakadsi M.
Hanner Martha
Leinert Ch.
Mistrik I.
Planck B.
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